Instant · Precise · Universal
28 units available
6 categories total
To convert years to days: multiply by 365 (or 365.25 for average including leap years). To seconds: multiply by 31,536,000.
1 yr = 365 d = 8,760 h = 525,600 min = 31,536,000 s. A leap year has 366 days (31,622,400 s).
For example, 1 Year (365 days) (yr) = 365.999337 Day (Sidereal) (d (Sid)).
| Year (365 days) (yr) | Day (Sidereal) (d (Sid)) |
|---|---|
| 0.1 | 36.5999337 |
| 0.5 | 182.9996685 |
| 1 | 365.999337 |
| 2 | 731.9986741 |
| 5 | 1829.996685 |
| 10 | 3659.99337 |
| 25 | 9149.983426 |
| 50 | 18299.96685 |
| 100 | 36599.9337 |
| 500 | 182999.6685 |
| 1000 | 365999.337 |
The common year is a unit of time equal to 365 days, or 31,536,000 seconds.
1 yr = 365 d = 8,760 h = 525,600 min = 31,536,000 s. A leap year has 366 days (31,622,400 s).
To convert years to days: multiply by 365 (or 365.25 for average including leap years). To seconds: multiply by 31,536,000.
Age calculation, financial year reporting, contract durations, academic years, and historical timeline reference.
The year 2000 was a leap year (divisible by 400), but 1900 was not (divisible by 100 but not 400). The Gregorian rule fixes the calendar's drift to 1 day per 3,236 years.
Assuming every 4th year is a leap year — century years must be divisible by 400 (so 1900 wasn't a leap year).
Leap year rule: divisible by 4 = leap, UNLESS divisible by 100, UNLESS also divisible by 400. So 2000 was, 1900 wasn't.
The sidereal day is the time for Earth to rotate once relative to distant stars — approximately 23 hours, 56 minutes, and 4 seconds (86,164.0905 seconds).
1 sidereal day ≈ 23 h 56 min 4.09 s = 86,164.09 s. About 3 min 56 s shorter than a solar day.
To convert sidereal days to solar days: multiply by 0.99727. To hours: multiply by 23.9345.
Telescope pointing and tracking, satellite ground track calculations, and astronomical observation scheduling.
Because of the ~4-minute difference, the night sky shifts gradually — the same star appears at the same position about 4 minutes earlier each night.
Equating sidereal day with solar day. The ~4-minute difference accumulates — after 6 months, sidereal noon is at solar midnight.
Imagine Earth spinning AND orbiting: after one full spin (sidereal day), Earth has moved in its orbit, so the Sun hasn't quite returned to the same position — that takes ~4 more minutes.



© 2026 UntangleTools. All Rights Reserved.